The importance of realistic starting models for hydrodynamic simulations of stellar collisions

Astrophysical Journal

Volumn 484, Issue 1 PART II, 1997, Pages

  Sills, Alison ^a   Lombardi Jr , James C ^b,c  

^a YALE UNIVERSITY   (United States)

^b Cornell University ^*  (United States)

^c Department of Population Medicine and Diagnostic Sciences   (United States)

Author keywords

Hydrodynamics; Stars: evolution

Indexed keywords

EID: 21744456638     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/310772     Document Type: Article

References (7)

1. Benz, W., & Hills, J. G. 1987, ApJ, 323, 614
2. Goodman, J., & Hernquist, L. 1991, ApJ, 378, 637
3. Guenther, D. B., Demarque, P., Kim, Y.-C., & Pinsonneault, M. H. 1992, ApJ, 387, 372
4. Lombardi, J. C., Rasio, F. A., & Shapiro, S. L. 1996, ApJ, 468, 797
5. Rasio, F. A. 1991, Ph.D. thesis, Cornell Univ.
6. Sandquist, E., Bolte, M., & Hernquist, L. 1997, ApJ, 477, 335
7. Sills, A., Lombardi, J. C., Bailyn, C. D., Demarque, P., Rasio, F. A., & Shapiro, S. L. 1997, ApJ, in press